Table 2: Structural properties of the dwarfsa; see also the discussion of individual objects.
Name Band $\mu_{E,0}$ $\alpha $ $m_{\rm LSB}^{\rm fit}$ $P_{\rm iso}$ $m_{P_{\rm iso}}$ $E_{\rm iso}$ $m_{\rm E_{\rm iso}}$ $m_{\rm SBP}$ $m_{\rm tot}$ $r_{\rm eff}$,r80 $\eta _{\rm ~SBP}$
(b, q)b   mag/ $\sq\hbox{$^{\prime\prime}$ }$ kpc mag kpc mag kpc mag mag mag kpc  
$\eta _{\rm LSB}^c$                        
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
Tol 3e J 18.24 $\pm$ 0.05 0.52 $\pm$ 0.01 11.78 1.20 12.42 2.29 11.86 11.31 11.29 0.61,1.23 1.45
$\star$ H 17.74 $\pm$ 0.06 0.53 $\pm$ 0.01 11.26 1.18 11.76 2.07 11.37 10.73 10.69 0.61,1.22 1.43
  $K_{\rm s}$ 17.45 $\pm$ 0.09 0.51 $\pm$ 0.01 11.06 1.18 11.48 2.12 11.15 10.50 10.46 0.57,1.15 1.49
Haro 14f J 17.46 $\pm$ 0.12 0.37 $\pm$ 0.01 12.70 1.39 12.45 1.88 12.82 11.81 11.78 0.61,1.21 1.18
3.6, 0.94 H 16.97 $\pm$ 0.26 0.39 $\pm$ 0.02 12.11 1.37 11.69 1.76 12.31 11.12 11.07 0.61,1.22 1.25
0.49 K' 16.88 $\pm$ 0.94 0.39 $\pm$ 0.08 11.99 1.32 11.54 1.83 12.17 10.98 10.97 0.60,1.21 1.45
UM 461e J 19.37 $\pm$ 0.18 0.21 $\pm$ 0.01 15.56 0.42 16.19 0.69 15.88 15.09 15.04 0.34,0.57 1.96
2.3, 0.85 H 18.82 $\pm$ 0.25 0.21 $\pm$ 0.02 14.98 0.35 16.12 0.60 15.46 14.66 14.57 0.37,0.61 1.82
0.49 $K_{\rm s}$ 18.47 $\pm$ 0.79 0.19 $\pm$ 0.04 14.79 0.36 15.75 0.63 15.14 14.46 14.37 0.32,0.54 2.04
Henize 2-10e J 18.46 $\pm$ 0.03 0.67 $\pm$ 0.01 10.46 0.87 10.57 2.80 10.55 9.80 9.70 0.41,1.26 2.50
$\star$ H 17.75 $\pm$ 0.04 0.64 $\pm$ 0.01 9.85 0.78 9.94 2.51 9.96 9.17 9.13 0.40,1.22 2.44
  $K_{\rm s}$ 17.51 $\pm$ 0.03 0.62 $\pm$ 0.01 9.68 0.79 9.62 2.56 9.78 8.95 8.89 0.34,1.04 2.44
Tol 1400-411e J 18.29 $\pm$ 0.11 0.33 $\pm$ 0.01 11.18 0.69 12.67 1.41 11.32 10.99 10.91 0.60,0.98 2.04
3.0, 0.82 Hd 17.30 $\pm$ 0.14 0.27 $\pm$ 0.01 10.57 0.31 13.65 1.18 10.71 10.57 10.55 0.57,0.93 1.33
0.63 $K_{\rm s}$ 17.39 $\pm$ 0.09 0.30 $\pm$ 0.01 10.43 0.50 12.49 1.28 10.58 10.32 10.31 0.59,0.97 1.75
Pox 4e J 19.26 $\pm$ 0.15 0.86 $\pm$ 0.03 15.15 2.27 14.80 2.87 15.54 14.24 14.20 1.24,2.17 1.75
2.7, 0.90 Hd 19.10 $\pm$ 0.31 0.88 $\pm$ 0.07 14.95 2.18 14.35 1.79 16.10 13.85 13.81 1.27,2.15 1.45
0.42 $K_{\rm s}$d - - - - - - - 13.54 13.52 1.18,2.09 1.96
Pox 4 Be J 19.47 $\pm$ 0.40 0.29 $\pm$ 0.04 17.37 0.51 19.29 0.93 17.67 17.21 17.12 0.54,0.87 0.75
2.0, 0.80 Hd - - - - - - - 16.83 16.72 0.51,0.80 0.77
0.49 $K_{\rm s}$d - - - - - - - 16.75 16.52 0.47,0.69 0.75
Tol 65e J 19.58 $\pm$ 0.18 0.28 $\pm$ 0.02 17.25 0.43 17.47 0.82 17.79 16.57 16.55 0.37,0.80 1.59
2.7, 0.90 Hd - - - - - - - 16.23 16.30 0.42,0.84 -
0.46 $K_{\rm s}$d - - - - - - - 16.03 15.99 0.24,0.61 -
Tol 1214-277e,g Jd 19.16 $\pm$ 0.24 0.53 $\pm$ 0.03 18.05 0.75 18.56 1.69 18.55 17.46 17.41 0.86,1.83 1.89
3.3, 0.92 Hd - - - - - - - 17.22 17.26 1.15,1.90 -
0.48 $K_{\rm s}$d - - - - - - - 16.94 17.07 0.81,1.67 -
Mkn 178f J 20.62 $\pm$ 0.11 0.28 $\pm$ 0.01 12.94 0.39 14.36 0.62 13.41 12.78 12.70 0.34,0.57 1.27
$\star$ Hd 19.87 $\pm$ 0.18 0.26 $\pm$ 0.02 12.35 0.26 14.85 0.51 12.92 12.29 12.25 0.34,0.58 1.12
  K'd 19.92 $\pm$ 0.43 0.27 $\pm$ 0.04 12.31 0.36 14.00 0.52 12.91 12.13 12.01 0.36,0.58 0.97
Mkn 1329e J 19.25 $\pm$ 0.04 0.67 $\pm$ 0.01 12.81 0.99 14.61 2.32 13.01 12.64 12.60 1.12,1.97 1.01
1.6, 0.70 Hd 18.81 $\pm$ 0.01 0.71 $\pm$ 0.01 12.25 1.01 13.85 2.09 12.57 12.00 11.94 1.17,2.08 1.11
0.68 $K_{\rm s}$ 18.24 $\pm$ 0.06 0.60 $\pm$ 0.01 12.03 0.79 14.56 2.09 12.23 11.95 11.93 1.09,1.87 0.72
IC 4662e J 16.79 $\pm$ 0.24 0.15 $\pm$ 0.01 10.60 0.55 10.32 0.83 10.73 9.68 9.64 0.29,0.53 1.41
4.8, 0.97 H 16.61 $\pm$ 0.73 0.15 $\pm$ 0.02 10.36 0.58 9.64 0.69 10.66 9.15 9.05 0.29,0.52 1.37
0.48 $K_{\rm s}$d - - - - - - - 9.04 8.93 0.27,0.48 1.75
UM 448e J 20.55 $\pm$ 0.07 3.83 $\pm$ 0.10 13.48 4.26 12.50 8.66 13.92 12.17 12.15 1.28,3.63 2.33
$\star$ H 19.95 $\pm$ 0.17 4.02 $\pm$ 0.31 12.77 4.08 11.88 7.60 13.39 11.52 11.50 1.32,3.94 2.40
  $K_{\rm s}$ 19.55 $\pm$ 0.15 3.61 $\pm$ 0.19 12.61 4.01 11.53 8.16 13.05 11.22 11.30 1.21,3.24 2.44
a: All values are corrected for Galactic extinction, adopting the AB from Table 1 (cf. Sect. 2.4.2).
b,c: See Sect. 3.2 for details. Objects whose LSB component has been modelled by a pure exponential fit (Eq. (5)) are marked with an asterisk.
d: Decomposition uncertainty higher (faint object, or data affected by nearby bright stars).
e: Calibration obtained at the ESO NTT, cf. Sect. 2.4.
f: Calibrated using field stars from the 2MASS catalogue, cf. Sect. 2.4.
g: Fit radius interval and (b, q) adopted from F01.

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